{"id":781,"date":"2015-05-07T18:09:33","date_gmt":"2015-05-07T18:09:33","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/soker\/?p=781"},"modified":"2015-05-07T18:19:19","modified_gmt":"2015-05-07T18:19:19","slug":"rescuing-the-intracluster-medium-of-ngc-5813","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/soker\/rescuing-the-intracluster-medium-of-ngc-5813\/","title":{"rendered":"Rescuing the intracluster medium of NGC 5813 (May 2015b)"},"content":{"rendered":"<p><strong>Shlomi Hi<img loading=\"lazy\" decoding=\"async\" class=\"  wp-image-784 alignleft\" src=\"http:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/05\/zShlomi2015.jpg\" alt=\"zShlomi2015\" width=\"219\" height=\"196\" srcset=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/05\/zShlomi2015.jpg 521w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2015\/05\/zShlomi2015-300x268.jpg 300w\" sizes=\"auto, (max-width: 219px) 100vw, 219px\" \/>llel<\/strong> (PhD Student), <strong>Assaf Sternberg<\/strong> and I argue that the intracluster medium\u00a0 (ICM) of the cooling flow galaxy group NGC 5813 is more likely to be heated by mixing of\u00a0post-shock jets&#8217; gas residing in hot bubbles with the ICM, than by shocks or turbulent-heating.\u00a0<span style=\"color: #800080\">Heating by mixing<\/span> rescues the outer ICM of NGC 5813 from its predestined fate according to\u00a0<span style=\"line-height: 1.5\">cooling flow feedback scenarios that are based on heating by shocks. \u00a0See\u00a0<\/span><a style=\"line-height: 1.5\" href=\"http:\/\/adsabs.harvard.edu\/abs\/2015arXiv150407754S\" target=\"_blank\">Paper.<\/a><\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Shlomi Hillel (PhD Student), Assaf Sternberg and I argue that the intracluster medium\u00a0 (ICM) of the cooling flow galaxy group NGC 5813 is more likely to be heated by mixing of\u00a0post-shock jets&#8217; gas residing in hot bubbles with the ICM, than by shocks or turbulent-heating.\u00a0Heating by mixing rescues the outer ICM of NGC 5813 from &hellip;<\/p>\n","protected":false},"author":6,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[2],"tags":[],"class_list":{"0":"post-781","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-news","7":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Rescuing the intracluster medium of NGC 5813 (May 2015b) Prof. Noam Soker<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/phsites.technion.ac.il\/soker\/rescuing-the-intracluster-medium-of-ngc-5813\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Rescuing the intracluster medium of NGC 5813 (May 2015b) Prof. Noam Soker\" \/>\n<meta property=\"og:description\" content=\"Shlomi Hillel (PhD Student), Assaf Sternberg and I argue that the intracluster medium\u00a0 (ICM) of the cooling flow galaxy group NGC 5813 is more likely to be heated by mixing of\u00a0post-shock jets&#8217; gas residing in hot bubbles with the ICM, than by shocks or turbulent-heating.\u00a0Heating by mixing rescues the outer ICM of NGC 5813 from &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/soker\/rescuing-the-intracluster-medium-of-ngc-5813\/\" \/>\n<meta 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